Skoči na glavni sadržaj

Central European Astrophysical Bulletin, Vol. 38 No. 1, 2014.

Izlaganje sa skupa

Parallelization of the SIR code

Thonhofer Stefan ; IGAM/Institute of Physics, University of Graz, Graz, Austria
L. R. Bellot-Rubio ; Instituto de Astrofísica de Andalucía (CSIC), Granada, Espana
Dominik Utz ; IGAM/Institute of Physics, University of Graz, Graz, Austria
Jan Jurčak ; Astronomical Institute CAS, Ondřejov, Czech Republic
Arnold Hanslmeier ; IGAM/Institute of Physics, University of Graz, Graz, Austria
I. Piantschitsch ; IGAM/Institute of Physics, University of Graz, Graz, Austria
J. Pauritsch ; IGAM/Institute of Physics, University of Graz, Graz, Austria
Birgit Lemmerer ; IGAM/Institute of Physics, University of Graz, Graz, Austria
S. Guttenbrunner ; IGAM/Institute of Physics, University of Graz, Graz, Austria

Puni tekst: engleski pdf 145 Kb

str. 31-37

preuzimanja: 375

citiraj

Sažetak

A high-resolution 3-dimensional model of the photospheric magnetic field is essential for the investigation of small-scale
solar magnetic phenomena. The SIR code is an advanced Stokes-inversion code that deduces physical quantities, e.g. magnetic
field vector, temperature, and LOS velocity, from spectropolarimetric data. We extended this code by the capability of directly
using large data sets and inverting the pixels in parallel. Due to this parallelization it is now feasible to apply the code
directly on extensive data sets. Besides, we included the possibility to use different initial model atmospheres for the
inversion, which enhances the quality of the results.

Ključne riječi

photosphere; spectropolarimetry; magnetic field

Hrčak ID:

143582

URI

https://hrcak.srce.hr/143582

Datum izdavanja:

20.11.2014.

Posjeta: 959 *